Similar to Figure 12, but instead we plot the conserved current profiles at a fixed radius r = 10r_g for all simulations in the library. The outward transport of angular momentum and energy in the jet strongly depends on the black hole spin for the MAD models. Negative values of ﹩\sqrt{-g}{J}_{L}^{r}﹩ at higher latitudes for the retrograde models are simply a reflection of the magnetic field lines and plasma in the jet corotating with the black hole.